Cosmological constraints from H  ii starburst galaxy apparent magnitude and other cosmological measurements

Cao, Shulei; Ryan, Joseph; Ratra, Bharat

doi:10.1093/mnras/staa2190

Title: Cosmological constraints from H ii starburst galaxy apparent magnitude and other cosmological measurements

Journal Article · Mon Jul 27 00:00:00 EDT 2020 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/staa2190· OSTI ID:1647480

^[1]; Ryan, Joseph ^[1]; Ratra, Bharat ^[1]

Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66502, USA

We use HII starburst galaxy apparent magnitude measurements to constrain cosmological parameters in six cosmological models. A joint analysis of H II galaxy, quasar angular size, baryon acoustic oscillations peak length scale, and Hubble parameter measurements result in relatively model-independent and restrictive estimates of the current values of the non-relativistic matter density parameter $$\Omega _{\rm m_0}$$ and the Hubble constant H₀. These estimates favour a 2.0–3.4σ (depending on cosmological model) lower H₀ than what is measured from the local expansion rate. The combined data are consistent with dark energy being a cosmological constant and with flat spatial hypersurfaces, but do not strongly rule out mild dark energy dynamics or slightly non-flat spatial geometries.

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Research Organization:: Kansas State Univ., Manhattan, KS (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0019038; SC0011840

OSTI ID:: 1647480

Alternate ID(s):: OSTI ID: 1802267

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Vol. 497 Journal Issue: 3; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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The H ii galaxy Hubble diagram strongly favours R _h = ct over ΛCDM Wei, Jun-Jie; Wu, Xue-Feng; Melia, Fulvio Monthly Notices of the Royal Astronomical Society, Vol. 463, Issue 2 https://doi.org/10.1093/mnras/stw2057	journal	August 2016

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